Isna Comparison Table

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Next Antarctic meteorite: LEW 85332 Up: Antarctic meteorite, CO chondrite, meteorite find Previous Antarctic meteorite: EETA 79001

Isna comparison table

Subject has sediment mechanism has weather resistance has metal abundance has part mean Ni content of sulfide has age has refractory inclusion abundance is an instance of has olivine and low Ca pyroxene homogeneity has distinguishing feature has part feldspar has part metal maximum bulk has fragmentation probability has fall location has name has chondrule glass type has weather has homogeneity of olivine and low Ca pyroxene has chondrule abundance has relative abundance has part chondrule has degree of aqueous alteration has abundance has prototype has petrologic subtype has value has total mass of find has structural state of low Ca pyroxene has peak temperature has parent body has part matrix has degree of thermal metamorphism has petrologic type range has matrix abundance has fall coordinate has part carbon has petrologic type has part maximum bulk Ni in metal is a kind of has find date has part water has image has number of find has ablative mass loss has definition has chondrule mean diameter has part sulfide Ni content

Antarctic meteorite which depends on its composition during meteor phase which depends on composition indicated by letters in the beginning of name 3 or 4 letter contracted from find location then last two digits of year then id number 485755 kg in degrees, minutes and seconds of lattitude and longitude meteorite recovery year is first 2 numbers in name 1691 directly proportional to initial velocity

CO chondrite agglomeration of particles, many of which record individual, diverse histories low 1 to 5 % by volume in weight % oldest and most primitive rock in solar system 13 % by volume greater than 5 % deviations elemental carbon minor primary grains only in weight % high because it is more friable than iron meteorite strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity based on the locale, region, or nearby town in which the fall occurred clear, isotropic, variable abundance definition goes here 48 % by volume 8 % of meteorite falls chondrules very sharply defined none rare relative to other chondrite types Ornans meteorite 2577 kg predominantly monoclinic less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter clastic and minor opaque none which depends on degree of aqueous alteration and thermal metamorphism 34 % by volume in degrees, minutes and seconds of lattitude and longitude 0.2 to 1 % by weight 3 greater than 20 % by weight, kamacite and taenite in exsolution relationship type 3 chondrite 0.3 to 3 % by weight 36 high because it is more friable than iron meteorite 0.15 millimeters less than 0.5 % by weight

meteorite find which depends on its composition during meteor phase which depends on composition strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity based on the locale, region, or nearby town in which the fall occurred can be severe due to long exposure time to environmental corrosion agents lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude meteorite when the meteorite was found 1691 directly proportional to initial velocity a meteorite whose fall was not witnessed

Isna agglomeration of particles, many of which record individual, diverse histories which depends on its composition 1 to 5 % by volume in weight % oldest and most primitive rock in solar system 13 % by volume Antarctic meteorite greater than 5 % deviations elemental carbon minor primary grains only in weight % during meteor phase which depends on composition Nile River near Luxor, Egypt Isna clear, isotropic, variable abundance can be severe due to long exposure time to environmental corrosion agents definition goes here 48 % by volume chondrules very sharply defined none rare relative to other chondrite types Ornans meteorite 3.7 lower because the fall was not witnessed 485755 kg predominantly monoclinic less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter clastic and minor opaque none which depends on degree of aqueous alteration and thermal metamorphism 34 % by volume 24° 50' N., 31° 40' E. 0.2 to 1 % by weight 3 greater than 20 % by weight, kamacite and taenite in exsolution relationship 1970 0.3 to 3 % by weight
1691 directly proportional to initial velocity 0.15 millimeters less than 0.5 % by weight

Next Antarctic meteorite: LEW 85332 Up: Antarctic meteorite, CO chondrite, meteorite find Previous Antarctic meteorite: EETA 79001

Subject	has sediment mechanism	has weather resistance	has metal abundance	has part mean Ni content of sulfide	has age	has refractory inclusion abundance	is an instance of	has olivine and low Ca pyroxene homogeneity	has distinguishing feature	has part feldspar	has part metal maximum bulk	has fragmentation probability	has fall location	has name	has chondrule glass type	has weather	has homogeneity of olivine and low Ca pyroxene	has chondrule abundance	has relative abundance	has part chondrule	has degree of aqueous alteration	has abundance	has prototype	has petrologic subtype	has value	has total mass of find	has structural state of low Ca pyroxene	has peak temperature	has parent body	has part matrix	has degree of thermal metamorphism	has petrologic type range	has matrix abundance	has fall coordinate	has part carbon	has petrologic type	has part maximum bulk Ni in metal	is a kind of	has find date	has part water	has image	has number of find	has ablative mass loss	has definition	has chondrule mean diameter	has part sulfide Ni content
Antarctic meteorite		which depends on its composition										during meteor phase which depends on composition	indicated by letters in the beginning of name	3 or 4 letter contracted from find location then last two digits of year then id number												485755 kg								in degrees, minutes and seconds of lattitude and longitude				meteorite	recovery year is first 2 numbers in name			1691	directly proportional to initial velocity
CO chondrite	agglomeration of particles, many of which record individual, diverse histories	low	1 to 5 % by volume	in weight %	oldest and most primitive rock in solar system	13 % by volume		greater than 5 % deviations	elemental carbon	minor primary grains only	in weight %	high because it is more friable than iron meteorite	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	based on the locale, region, or nearby town in which the fall occurred	clear, isotropic, variable abundance		definition goes here	48 % by volume	8 % of meteorite falls	chondrules very sharply defined	none	rare relative to other chondrite types	Ornans meteorite			2577 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	clastic and minor opaque	none	which depends on degree of aqueous alteration and thermal metamorphism	34 % by volume	in degrees, minutes and seconds of lattitude and longitude	0.2 to 1 % by weight	3	greater than 20 % by weight, kamacite and taenite in exsolution relationship	type 3 chondrite		0.3 to 3 % by weight		36	high because it is more friable than iron meteorite		0.15 millimeters	less than 0.5 % by weight
meteorite find		which depends on its composition										during meteor phase which depends on composition	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	based on the locale, region, or nearby town in which the fall occurred		can be severe due to long exposure time to environmental corrosion agents									lower because the fall was not witnessed	485755 kg								in degrees, minutes and seconds of lattitude and longitude				meteorite	when the meteorite was found			1691	directly proportional to initial velocity	a meteorite whose fall was not witnessed
Isna	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	1 to 5 % by volume	in weight %	oldest and most primitive rock in solar system	13 % by volume	Antarctic meteorite	greater than 5 % deviations	elemental carbon	minor primary grains only	in weight %	during meteor phase which depends on composition	Nile River near Luxor, Egypt	Isna	clear, isotropic, variable abundance	can be severe due to long exposure time to environmental corrosion agents	definition goes here	48 % by volume		chondrules very sharply defined	none	rare relative to other chondrite types	Ornans meteorite	3.7	lower because the fall was not witnessed	485755 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	clastic and minor opaque	none	which depends on degree of aqueous alteration and thermal metamorphism	34 % by volume	24° 50' N., 31° 40' E.	0.2 to 1 % by weight	3	greater than 20 % by weight, kamacite and taenite in exsolution relationship		1970	0.3 to 3 % by weight		1691	directly proportional to initial velocity		0.15 millimeters	less than 0.5 % by weight